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Lightning current and luminosity at and above channel bottom for return strokes and M‐components
Author(s) -
Carvalho F. L.,
Uman M. A.,
Jordan D. M.,
Ngin T.
Publication year - 2015
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
eISSN - 2169-8996
pISSN - 2169-897X
DOI - 10.1002/2015jd023814
Subject(s) - luminosity , physics , peak current , current (fluid) , astrophysics , amplitude , lightning (connector) , optics , electrode , power (physics) , quantum mechanics , galaxy , electrochemistry , thermodynamics
We measured current and luminosity at the channel bottom of 12 triggered lightning discharges including 44 return strokes, 23 M‐components, and 1 initial continuous current pulse. Combined current and luminosity data for impulse currents span a 10–90% risetime range from 0.15 to 192 µs. Current risetime and luminosity risetime at the channel bottom are roughly linearly correlated ( τ r , I = 0.71 τ r , L 1.08 ). We observed a time delay between current and the resultant luminosity at the channel bottom, both measured at 20% of peak amplitude, that is approximately linearly related to both the luminosity 10–90% risetime (Δ t 20, b = 0.24 τ r , L 1.12 ) and the current 10–90% risetime (Δ t 20, b = 0.35 τ r , I 1.03 ). At the channel bottom, the peak current is roughly proportional to the square root of the peak luminosity ( I P = 21.89 L P 0.57 ) over the full range of current and luminosity risetimes. For two return strokes we provide measurements of stroke luminosity vs. time for 11 increasing heights to 115 m altitude. We assume that measurements above the channel bottom behave similarly to those at the bottom and find that (1) one return stroke current peak decayed at 115 m to about 47% of its peak value at channel bottom, while the luminosity peak at 115 m decayed to about 20%, and for the second stroke 38% and 12%, respectively; and (2) measured upward return stroke luminosity speeds of the two strokes of 1.10 × 10 8 and 9.7 × 10 7 ms −1 correspond to current speeds about 30% faster. These results represent the first determination of return stroke current speed and current peak value above ground derived from measured return stroke luminosity data.